Search Publications

A Chandra X-ray Observatory Study of PSR J1740-5340 and Candidate Millisecond Pulsars in the Globular Cluster NGC 6397
DOI: 10.1088/0004-637X/709/1/241 Bibcode: 2010ApJ...709..241B

Bogdanov, Slavko; Heinke, Craig O.; Cohn, Haldan N. +3 more

We present a deep Chandra X-ray Observatory study of the peculiar binary radio millisecond pulsar (MSP) PSR J1740-5340 and candidate millisecond pulsars in the globular cluster NGC 6397. The X-rays from PSR J1740-5340 appear to be non-thermal and exhibit variability at the binary period. These properties suggest the presence of a relativistic intr…

2010 The Astrophysical Journal
eHST 66
Specular reflection on Titan: Liquids in Kraken Mare
DOI: 10.1029/2009GL042312 Bibcode: 2010GeoRL..37.7104S

Sotin, Christophe; Barnes, Jason W.; Soderblom, Jason M. +12 more

After more than 50 close flybys of Titan by the Cassini spacecraft, it has become evident that features similar in morphology to terrestrial lakes and seas exist in Titan's polar regions. As Titan progresses into northern spring, the much more numerous and larger lakes and seas in the north-polar region suggested by Cassini RADAR data, are becomin…

2010 Geophysical Research Letters
Cassini 66
Magnetic Bright Points in the Quiet Sun
DOI: 10.1088/2041-8205/715/1/L26 Bibcode: 2010ApJ...715L..26S

Sánchez Almeida, J.; Del Moro, D.; Bonet, J. A. +1 more

We present a visual determination of the number of bright points (BPs) existing in the quiet Sun, which are structures though to trace intense kG magnetic concentrations. The measurement is based on a 0farcs1 angular resolution G-band movie obtained with the Swedish Solar Telescope at the solar disk center. We find 0.97 BPs Mm-2, which …

2010 The Astrophysical Journal
Hinode 66
INTEGRAL results on supergiant fast X-ray transients and accretion mechanism interpretation: ionization effect and formation of transient accretion discs
DOI: 10.1111/j.1365-2966.2010.17216.x Bibcode: 2010MNRAS.408.1540D

Sidoli, L.; Ducci, L.; Paizis, A.

We performed a systematic analysis of all INTEGRAL observations from 2003 to 2009 of 14 supergiant fast X-ray transients (SFXTs), implying a net exposure time of about 30 Ms. For each source we obtained light curves and spectra (3-100 keV), discovering several new outbursts. We discuss the X-ray behaviour of SFXTs emerging from our analysis in the…

2010 Monthly Notices of the Royal Astronomical Society
INTEGRAL 66
Earth-Moon-Mars Radiation Environment Module framework
DOI: 10.1029/2009SW000523 Bibcode: 2010SpWea...8.0E02S

Schwadron, N. A.; Posner, A.; Dayeh, M. A. +11 more

We are preparing to return humans to the Moon and setting the stage for exploration to Mars and beyond. However, it is unclear if long missions outside of low-Earth orbit can be accomplished with acceptable risk. The central objective of a new modeling project, the Earth-Moon-Mars Radiation Exposure Module (EMMREM), is to develop and validate a nu…

2010 Space Weather
Ulysses 66
The reversal of the rotational modulation rates of the north and south components of Saturn kilometric radiation near equinox
DOI: 10.1029/2010GL045796 Bibcode: 2010GeoRL..3724101G

Gurnett, D. A.; Persoon, A. M.; Kurth, W. S. +5 more

It has been known for many years that Saturn emits intense radio emissions at kilometer wavelengths and that this radiation is modulated by the rotation of the planet at a rate that varies slowly on time scales of years. Recently it has been shown that the radio emission consists of two components that have different rotational modulation rates, o…

2010 Geophysical Research Letters
Cassini Ulysses 66
Multispacecraft observation of electron pitch angle distributions in magnetotail reconnection
DOI: 10.1029/2009JA014553 Bibcode: 2010JGRA..115.1209W

Wang, Shui; Huang, Can; Lu, Quanming +1 more

In this paper, we present Cluster observations of a magnetotail reconnection event without the presence of an obvious guide magnetic field and analyze electron pitch angle distributions in the vicinity of the X line and the outflow region, respectively. In the vicinity of the X line, at lower energies the distributions are highly anisotropic (fiel…

2010 Journal of Geophysical Research (Space Physics)
Cluster DoubleStar 66
Evolution of the Solar Activity Over Time and Effects on Planetary Atmospheres. II. κ1 Ceti, an Analog of the Sun when Life Arose on Earth
DOI: 10.1088/0004-637X/714/1/384 Bibcode: 2010ApJ...714..384R

Ribas, I.; de Medeiros, J. R.; Porto de Mello, G. F. +6 more

The early evolution of Earth's atmosphere and the origin of life took place at a time when physical conditions at the Earth were radically different from its present state. The radiative input from the Sun was much enhanced in the high-energy spectral domain, and in order to model early planetary atmospheres in detail, a knowledge of the solar rad…

2010 The Astrophysical Journal
eHST 66
Spectral variability and reverberation time delays in the Suzaku X-ray spectrum of NGC 4051
DOI: 10.1111/j.1365-2966.2009.16149.x Bibcode: 2010MNRAS.403..196M

Turner, T. J.; Kraemer, S. B.; Crenshaw, D. M. +3 more

Long-exposure Suzaku X-ray observations of the nearby active galaxy NGC 4051 from 2005 and 2008 are analysed, in an attempt to reach a self-consistent understanding of both the spectral variability on long time-scales and the broad-band variability at high time resolution. The techniques of principal components analysis and a maximum likelihood me…

2010 Monthly Notices of the Royal Astronomical Society
Suzaku 66
The baryonic content and Tully-Fisher relation at z ~ 0.6
DOI: 10.1051/0004-6361/200912081 Bibcode: 2010A&A...510A..68P

Yang, Y.; Flores, H.; Hammer, F. +3 more

Context. Using the multi-integral-field spectrograph GIRAFFE at VLT, we previsouly derived the stellar-mass Tully-Fisher Relation (smTFR) at z ~ 0.6 for a representative sample of 63 emission-line galaxies. We found that the distant relation is systematically offset by roughly a factor of two toward lower masses from the local relation.
Aims:…

2010 Astronomy and Astrophysics
eHST 66